Showing 21–40 of 44 results
/ Date/ Name
Jul 3, 2019Final Release of the OGLE Collection of Cepheids and RR Lyrae Stars in the Magellanic System. The Outer RegionsApr 17, 2019OGLE-ing the Magellanic System: Cepheids in the BridgeApr 16, 2019OGLE-ing the Magellanic System: RR Lyrae Stars in the BridgeOct 27, 2017OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf BoundarySep 21, 2016The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)cJan 7, 2016Spitzer Observations of OGLE-2015-BLG-1212 Reveal a New Path to Breaking Strong Microlens DegeneraciesOct 14, 2015The frequency of snowline-region planets from four-years of OGLE-MOA-Wise second-generation microlensingAug 26, 2015Spitzer Microlens Measurement of a Massive Remnant in a Well-Separated BinaryJul 9, 2015A Venus-Mass Planet Orbiting a Brown Dwarf: Missing Link between Planets and MoonsNov 26, 2014Pathway to the Galactic Distribution of Planets: Combined Spitzer and Ground-Based Microlens Parallax Measurements of 21 Single-Lens EventsJul 4, 2014A Terrestrial Planet in a ~1 AU Orbit Around One Member of a ~15 AU BinaryMar 12, 2014Candidate Gravitational Microlensing Events for Future Direct Lens ImagingOct 9, 2013A Super-Jupiter orbiting a late-type star: A refined analysis of microlensing event OGLE-2012-BLG-0406Sep 30, 2013MOA-2010-BLG-328Lb: a sub-Neptune orbiting very late M dwarf ?Jul 15, 2013Super-massive planets around late-type stars - the case of OGLE-2012-BLG-0406LbNov 16, 2012MOA-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf BoundaryApr 13, 2012Characterizing Low-Mass Binaries From Observation of Long Time-scale Caustic-crossing Gravitational Microlensing EventsSep 15, 2011Microlensing Binaries Discovered through High-Magnification ChannelApr 27, 2011OGLE-2005-BLG-018: Characterization of Full Physical and Orbital Parameters of a Gravitational Binary LensMay 6, 2010OGLE 2008--BLG--290: An accurate measurement of the limb darkening of a Galactic Bulge K Giant spatially resolved by microlensing